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Proceedings Article

The dark energy survey and operations: years 1 to 3

H. T. Diehl ; E. Neilsen ; R. Gruendl ; B. Yanny ; T. M. C. Abbott ; J. Aleksić ; S. Allam ; J. Annis ; E. Balbinot ; M. Baumer ; L. Beaufore ; K. Bechtol ; G. Bernstein ; S. Birrer ; C. Bonnett ; D. Brout ; C. Bruderer ; E. J. Buckley-Geer ; D. Capozzi ; A. Carnero Rosell ; F. J. Castander ; R. Cawthon ; C. Chang ; L. Clerkin ; R. Covarrubias ; C. Cuhna ; C. D'Andrea ; L. da Costa ; R. Das ; C. Davis ; J. Dietrich ; A. Drlica-Wagner ; A. Elliott ; T. F. Eifler ; J. Etherington ; B. L. Flaugher ; J. Frieman ; A. Fausti Neto ; M. G. Fernández ; C. Furlanetto ; D. Gangkofner ; D. W. Gerdes ; D. A. Goldstein ; K. Grabowski ; R. R. Gupta ; S. Hamilton ; H. Head ; J. Helsby ; D. Hollowood ; K. Honscheid ; D. James ; M. Johnson ; M. W. G. Johnson ; S. Jouvel ; T. Kacprzac ; S. Kent ; R. Kessler ; A. Kim ; E. Krause ; C. I. Krawiec ; A. Kremin ; R. Kron ; S. Kuhlmann ; N. Kuropatkin ; O. Lahav ; J. Lasker ; T. S. Li ; E. Luque ; N. Maccrann ; M. March ; J. Marshall ; N. P. Mondrik ; E. P. Morganson ; D. Mudd ; A. Nadolski ; P. Nugent ; P. Melchior ; F. Menanteau ; D. Q. Nagasawa ; B. Nord ; R. Ogando ; L. Old ; A. Palmese ; D. Petravick ; A. A. Plazas ; A. Pujol ; A. B. A. Queiroz ; K. Reil ; A. K. Romer ; R. Rosenfeld ; A. Roodman ; P. Rooney ; M. Sako ; A. I. Salvador ; C. Sánchez ; E. Sánchez Álvaro ; B. X. Santiago ; A. Schooneveld ; M. Schubnell ; E. Sheldon ; A. Smith ; R. C. Smith ; M. Soares-Santos ; F. Sobreira ; M. Soumagnac ; H. Spinka ; S. S. Tie ; D. Tucker ; V. Vikram ; K. Vivas ; A. R. Walker ; W. Wester ; M. Wiesner ; H. Wilcox ; P. Williams ; A. Zenteno ; Y. Zhang ; Z. Zhang
[+] Author Affiliations
H. T. Diehl, E. Neilsen, B. Yanny, S. Allam, J. Annis, E. J. Buckley-Geer, A. Drlica-Wagner, B. L. Flaugher, J. Frieman, K. Grabowski, S. Kent, R. Kron, N. Kuropatkin, B. Nord, M. Soares-Santos, F. Sobreira, D. Tucker, W. Wester, M. Wiesner, Y. Zhang

Fermi National Accelerator Lab. (United States)

R. Gruendl, R. Covarrubias, M. Johnson, M. W. G. Johnson, E. P. Morganson, F. Menanteau, D. Petravick

National Ctr. for Supercomputing Applications (United States)

T. M. C. Abbott, D. James, R. C. Smith, K. Vivas, A. R. Walker, A. Zenteno

National Optical Astronomy Observatory, Cerro Tololo Inter-American Observatory (Chile)

J. Aleksić, C. Bonnett, C. Sánchez

The Barcelona Institute of Science and Technology (Spain)

E. Balbinot

Univ. of Surrey (United Kingdom)

M. Baumer

Stanford Univ. (United States)

L. Beaufore, A. Elliott, K. Honscheid, D. Mudd, S. S. Tie

The Ohio State Univ. (United States)

K. Bechtol, R. Cawthon, J. Helsby, R. Kessler, J. Lasker, P. Williams

Kavli Institute for Cosmological Physics (United States)

G. Bernstein, D. Brout, T. F. Eifler, E. Krause, C. I. Krawiec, M. March, M. Sako

Univ. of Pennsylvania (United States)

S. Birrer, C. Bruderer, C. Chang

ETH Zurich (Switzerland)

D. Capozzi, A. Carnero Rosell, C. D'Andrea, H. Wilcox

Univ. of Portsmouth (United Kingdom)

F. J. Castander, M. G. Fernández, A. Pujol

Institut de Ciéncies de l’Espai (Spain)

L. Clerkin, S. Jouvel, T. Kacprzac, O. Lahav, A. Palmese, M. Soumagnac

Univ. College London (United Kingdom)

C. Cuhna, C. Davis, K. Reil, A. Roodman

Kavli Institute for Particle Astrophysics and Cosmology (United States)

L. da Costa, A. Fausti Neto, R. Ogando

Lab. Interinstitucional de e-Astronomia (Brazil)

R. Das, D. W. Gerdes, S. Hamilton, A. Kremin, M. Schubnell

Univ. of Michigan (United States)

J. Dietrich, D. Gangkofner

Univ. Observatory Munich (Germany)

J. Etherington

Univ. of Portsmouth (United States)

C. Furlanetto

Univ. of Notingham (United Kingdom)

D. A. Goldstein, A. Kim, P. Nugent

Lawrence Berkeley National Lab. (United States)

R. R. Gupta, S. Kuhlmann, H. Spinka, V. Vikram

Argonne National Lab. (United States)

H. Head, A. Smith

Austin Peay State Univ. (United States)

D. Hollowood

Univ. of California, Santa Cruz (United States)

T. S. Li, J. Marshall, N. P. Mondrik, D. Q. Nagasawa

Texas A&M Univ. (United States)

E. Luque, A. B. A. Queiroz, B. X. Santiago

Instituto de Física, UFRGS (Brazil)

N. Maccrann

Jodrell Bank Ctr. for Astrophysics (United Kingdom)

A. Nadolski

Univ. of Illinois at Urbana-Champaign (United States)

P. Melchior

Excellence Cluster Universe (Germany)

L. Old

Univ. of Nottingham (United Kingdom)

A. A. Plazas, E. Sheldon

Brookhaven National Lab. (United States)

A. K. Romer, P. Rooney

Univ. of Sussex (United Kingdom)

R. Rosenfeld

Instituto de Física Teórica, Univ. Estadual Paulista (Brazil)

A. I. Salvador

Instituto de Física Teórica, UAM-CSIC (Spain)

E. Sánchez Álvaro

Ctr. de Investigaciones Energéticas, Medioambientales y Tecnológicas (Spain)

A. Schooneveld

Univ. of Cambridge (United Kingdom)

Z. Zhang

SLAC National Accelerator Lab. (United States)

Proc. SPIE 9910, Observatory Operations: Strategies, Processes, and Systems VI, 99101D (July 15, 2016); doi:10.1117/12.2233157
Text Size: A A A
From Conference Volume 9910

  • Observatory Operations: Strategies, Processes, and Systems VI
  • Alison B. Peck; Robert L. Seaman; Chris R. Benn
  • Edinburgh, United Kingdom | June 26, 2016

abstract

The Dark Energy Survey (DES) is an operating optical survey aimed at understanding the accelerating expansion of the universe using four complementary methods: weak gravitational lensing, galaxy cluster counts, baryon acoustic oscillations, and Type Ia supernovae. To perform the 5000 sq-degree wide field and 30 sq-degree supernova surveys, the DES Collaboration built the Dark Energy Camera (DECam), a 3 square-degree, 570-Megapixel CCD camera that was installed at the prime focus of the Blanco 4-meter telescope at the Cerro Tololo Inter-American Observatory (CTIO). DES has completed its third observing season out of a nominal five. This paper describes DES “Year 1” (Y1) to “Year 3” (Y3), the strategy, an outline of the survey operations procedures, the efficiency of operations and the causes of lost observing time. It provides details about the quality of the first three season's data, and describes how we are adjusting the survey strategy in the face of the El Niño Southern Oscillation. © (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Citation

H. T. Diehl ; E. Neilsen ; R. Gruendl ; B. Yanny ; T. M. C. Abbott, et al.
" The dark energy survey and operations: years 1 to 3 ", Proc. SPIE 9910, Observatory Operations: Strategies, Processes, and Systems VI, 99101D (July 15, 2016); doi:10.1117/12.2233157; http://dx.doi.org/10.1117/12.2233157


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